An observational and theoretical view of the radial distribution of HI gas in galaxies

Monthly Notices of the Royal Astronomical Society

Volumn 441, Issue 3, 2014, Pages 2159-2172

  Wang, Jing ^a   Fu, Jian ^b   Aumer, Michael ^a,c   Kauffmann, Guinevere ^a   Józsa, Gyula I G ^d,e   Serra, Paolo ^f   Huang, Mei Ling ^a   Brinchmann, Jarle ^g   Van Der Hulst, Thijs ^h   Bigiel, Frank ⁱ  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c EXCELLENCE CLUSTER UNIVERSE   (Germany)

^d ASTRON   (Netherlands)

^e UNIVERSITY OF BONN   (Germany)

^f CSIRO   (Australia)

^g LEIDEN UNIVERSITY   (Netherlands)

^h UNIVERSITY OF GRONINGEN   (Netherlands)

ⁱ UNIVERSITY OF HEIDELBERG   (Germany)

Author keywords

Galaxies: Evolution; Galaxies: ISM; Galaxies: Spiral

Indexed keywords

EXPONENTIAL FUNCTIONS; GALAXIES; STARS;

ANALYTIC MODELING; DENSITY PROFILE; DISK GALAXIES; EMPIRICAL MODEL; GALAXIES: ISM; GALAXIES: SPIRALS; GALAXY EVOLUTION; RADIAL DISTRIBUTIONS; RADIAL PROFILES; SURFACE DENSITY;

ANALYTICAL MODELS;

EID: 84903160362     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu649     Document Type: Article

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